Neutrino Mass Sum Rules from Modular $\mathcal{A}_4$ Symmetry
Salvador Centelles Chuli\'a, Ranjeet Kumar, Oleg Popov, Rahul, Srivastava

TL;DR
This paper introduces a minimalistic model using modular $ ext{A}_4$ symmetry within a type-II seesaw framework, deriving a neutrino mass sum rule that constrains the absolute neutrino mass scale and has testable cosmological implications.
Contribution
It presents a novel minimalistic model with modular $ ext{A}_4$ symmetry that predicts a specific neutrino mass sum rule linking oscillation data to absolute mass scale.
Findings
Predicts total neutrino mass sum around 0.1 eV for both mass orderings.
Provides a testable relation that constrains neutrino mass parameters.
Implications for cosmology and neutrinoless double beta decay experiments.
Abstract
Modular symmetries offer a dynamic approach to understanding the flavour structure of leptonic mixing. Using the modular flavour symmetry integrated in a type-II seesaw, we propose a simple and minimalistic model that restricts the neutrino oscillation parameter space and, most importantly, introduces a sum rule in the physical neutrino masses. When combined with the mass squared differences observed in neutrino oscillations, this sum rule determines the absolute neutrino mass scale. This has significant implications for cosmology, neutrinoless double beta decay experiments and direct neutrino mass measurements. In particular, the model predicts eV for both normal and inverted ordering, and thus can be fully probed by the current generation of cosmological probes in the upcoming years.
Peer Reviews
No public reviews on file for this paper yet. If you reviewed it on a platform where reviews are public (OpenReview, ICLR, NeurIPS, ICML), you can paste yours below so the community can read it here.
Videos
No videos yet. Explain this paper in a talk, walkthrough, or lecture? Add one.
Taxonomy
TopicsNeutrino Physics Research · Particle physics theoretical and experimental studies · Astrophysics and Cosmic Phenomena
